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Coronae of nearby star clusters
We present a novel view on the morphology and dynamical state of ten prominent, nearby (<=500pc), and young (~30-300Myr) open star clusters with Gaia DR2: Per, Blanco 1, IC... -
PRM catalogue of halo MS stars
The Gaia mission has provided the largest ever astrometric chart of the Milky Way. Using it to map the Galactic halo is helpful for disentangling its merger history. The... -
Proper motion catalogue of Galactic Centre
Proper motion studies of stars in the centre of the Milky Way have typically been limited to the Arches and Quintuplet clusters, and to the central parsec. Here we present the... -
Binarity of Hipparcos stars from Gaia pm anomaly
The census of stellar and substellar companions of nearby stars is largely incomplete, in particular towards the low mass brown dwarf and long-period exoplanets. It is however... -
Multiwavelength study of Sgr A*
We present the results of the multiwavelength study of the flaring activity of the supermassive black hole named Sgr A is located at the dynamical center of the Milky Way. We... -
Na and Al abundances of 1303 stars
Stellar evolution models predict that internal mixing should cause some sodium overabundance at the surface of red giants more massive than ~1.5-2.0M_{aun}_. The surface... -
Continuum sources from the THOR survey
We carried out a large program with the Karl G. Jansky Very Large Array (VLA): "THOR: The HI, OH, Recombination line survey of the Milky Way". We observed a significant portion... -
Photometry of DBS 77-78-102-160-161 regions
We report a study of the global properties of some embedded clusters placed in the fourth quadrant of the MilkyWay to clarify some issues related with their location into de... -
Star formation in massive clumps in Milky Way
Newborn stars form within the localized, high density regions of molecular clouds. The sequence and rate at which stars form in dense clumps and the dependence on local and... -
47 Tuc red giants chemical composition
The study of chemical abundance patterns in globular clusters is of key importance to constrain the different candidates for intra-cluster pollution of light elements. We aim at... -
HI shells in the outer Milky Way
We present results of a method for an automatic search for HI shells in 3D data cubes and apply it to the Leiden-Dwingeloo HI survey of the northern Milky Way. In the 2nd...